Fluid-drops as cosmological models. II - Discontinuities in fluid-drop evaporation - A unified model for problems of stellar evolution, solar system origin and planetary geology

Details Fluid-drops as cosmological models. II - Discontinuities in fluid-drop evaporation - A unified model for problems of stellar evolution, solar system origin and planetary geology Fluid-drops as cosmological models. II - Discontinuities in fluid-drop evaporation - A unified model for problems of stellar evolution, solar system origin and planetary geology

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ssct....1..359d&link_type=abstract

Speculations in Science and Technology, vol. 1, Oct. 1978, p. 359-376.

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Cosmology, Drops (Liquids), Planetology, Solar System, Stellar Evolution, Earth-Moon System, Evaporation, Hertzsprung-Russell Diagram, Particulates, Planetary Evolution, Stellar Models

Scientific paper

The application of discontinuities in the evaporation of drops of fluid solutions as a unified model for stellar evolution and the origin of the solar system is discussed. It is found that sequential events in the process of drop evaporation from a glass slide have their homomorphic analogs repeated at various levels of astrophysical hierarchies. Stellar hydrogen and helium are represented by the solvent, heavier element particulates by the solute and intrinsically generated heat by the application of external heat. If applied to stellar evolution, the model would imply discrete discontinuous reductions in stellar mass and gravitation strength, from that of supergiant stars to dense dwarfs, including phases of implosion and contraction and the generation of planets from condensed sedimentation rings as the star pulsates. Planets thus formed would also undergo a series of pulsating contractions and implosions, creating satellites and rings.

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